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Volumn 550, Issue 1-2, 2002, Pages 117-120

Massive charged scalar field in a Reissner-Nordstrom black hole background: Quasinormal ringing

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; DECOMPOSITION; ELECTRICITY; ELECTROMAGNETIC FIELD; GEOMETRY; OSCILLATION; SIMULATION;

EID: 0037069771     PISSN: 03702693     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0370-2693(02)02974-X     Document Type: Article
Times cited : (111)

References (18)
  • 7
    • 0037104540 scopus 로고    scopus 로고
    • Note that QN behaviour of the SAdS black hole, unlike ordinary Schwarzshild BH, depends upon the horizon radius. The QNF is proprtional to the horizon radius for large black holes (and thereby proportional to the temperature) and goes to pure AdS modes when the horizon radius goes to zero, see also: R.A. Konoplya, Phys. Rev. D 66 (2002) 044009.
    • (2002) Phys. Rev. D , vol.66 , pp. 044009
    • Konoplya, R.A.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.